๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Contribution of Characteristic X-rays to the Radiation of Solar Flares

โœ Scribed by ACTON, LOREN W.


Book ID
109645421
Publisher
Nature Publishing Group
Year
1965
Tongue
English
Weight
246 KB
Volume
207
Category
Article
ISSN
0028-0836

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๐Ÿ“œ SIMILAR VOLUMES


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The polarization of hard solar X-radiation (> l0 keV) is calculated on the assumption that electrons get a non-isotropic velocity distribution in the initial phase of a flare. The bremsstrahlung generated by nonthermal electrons spiralling around magnetic field lines with discrete pitch angles is co

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The problem of producing the hard X-ray burst at the onset of solar flares may be thought of in terms of the problem of producing the non-thermal electrons which emit the X-rays via bremsstrahlung. Electron acceleration to relativistic energies without similar ion acceleration is difficult to achiev

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